1 00:00:12,150 --> 00:00:04,030 Music 2 00:00:12,170 --> 00:00:16,190 Narrator: Just to the east of M27, the "Apple Core" nebula, 3 00:00:16,210 --> 00:00:20,360 there's a star that can be seen in binoculars. And this star hosts 4 00:00:20,380 --> 00:00:24,460 a giant planet. The star is slightly smaller and 5 00:00:24,480 --> 00:00:28,510 cooler than our sun. In 2005, astronomers found it's Jupiter- 6 00:00:28,530 --> 00:00:32,600 size planet, named HD 189733b. 7 00:00:32,620 --> 00:00:36,610 Incredibly, the planet orbits just 3 million miles 8 00:00:36,630 --> 00:00:40,630 from the star, twelve times closer than Mercury orbits our sun. 9 00:00:40,650 --> 00:00:44,660 It's so close that the planet whips around its star in a little 10 00:00:44,680 --> 00:00:48,750 over two days. But this planet pays a steep price for skirting 11 00:00:48,770 --> 00:00:52,780 its sun. Sometimes, the star erupts with powerful flares, 12 00:00:52,800 --> 00:00:56,830 flares that heat the planet's upper atmosphere so much that the gasses 13 00:00:56,850 --> 00:01:00,840 simply escape. Since the planet passes in front if its 14 00:01:00,860 --> 00:01:04,890 star as we see it from Earth, astronomers were able to use the Hubble 15 00:01:04,910 --> 00:01:08,940 Space Telescope to establish that the atmosphere was evaporating. 16 00:01:08,960 --> 00:01:13,030 But when they looked again in 2010, there was not trace of an escaping 17 00:01:13,050 --> 00:01:17,070 atmosphere. Yet when astronomers looked once more in 2011, 18 00:01:17,090 --> 00:01:21,100 they saw dramatic evidence that the atmosphere was eroding. 19 00:01:21,120 --> 00:01:25,140 Hydrogen gas was rushing away from the planet at speeds over 300,000 miles 20 00:01:25,160 --> 00:01:29,160 an hour. What had changed? The same astronomers 21 00:01:29,180 --> 00:01:33,230 were also watching the star with NASA's Swift satellite. Just 8 hours before 22 00:01:33,250 --> 00:01:37,280 Hubble was scheduled to look for the planet's atmosphere, Swift saw the star 23 00:01:37,300 --> 00:01:41,330 erupt in a powerful X-ray flare. Similar 24 00:01:41,350 --> 00:01:45,370 flares happen frequently on the sun. But because the planet is so 25 00:01:45,390 --> 00:01:49,400 big and so close to its star, this X-ray blast had an outsized 26 00:01:49,420 --> 00:01:53,470 effect, heating the planet's atmosphere and sweeping away 1,000 27 00:01:53,490 --> 00:01:57,490 tons of gas each second. The escaping gas gave the planet a 28 00:01:57,510 --> 00:02:01,520 comet-like tail. While HD 189733b 29 00:02:01,540 --> 00:02:05,570 has plenty of gas to spare, atmospheric erosion is an 30 00:02:05,590 --> 00:02:09,580 important process, one able to whittle down any gas giant planet that 31 00:02:09,600 --> 00:02:13,630 hugs its star too close.